Evolution of Central Stars of Planetary Nebulae Towards the Crystallizing White Dwarf Stage

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The evolution of the central stars of planetary nebulae, interpreted as hot white dwarfs with liquefying cores, towards the cold white dwarf stage is discussed and theoretical (non-computational) evolutionary tracks are built for such central stars as they cool towards the crystallizing region. The conclusions seem to hint a picture in which crystalline white dwarfs can be looked at as final stages of the central stars of planetary nebulae.

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